Supermassive black hole binaries at high energies
An accretion disk around a supermassive black hole may be strongly perturbed by the presence of a secondary black hole. Recent simulations have shown that, under certain conditions, the tidal torques exerted by the secondary black hole may open an annular gap in the disk. In this regime, matter &quo...
Guardado en:
| Autores principales: | Romero, Gustavo Esteban, Pérez, Daniela, Vila, Gabriela Soledad |
|---|---|
| Formato: | Articulo |
| Lenguaje: | Inglés |
| Publicado: |
2014
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| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/139193 |
| Aporte de: |
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